Dark Energy Stars
Conference
·
OSTI ID:15011619
Event horizons and closed time-like curves cannot exist in the real world for the simple reason that they are inconsistent with quantum mechanics. Following ideas originated by Robert Laughlin, Pawel Mazur, Emil Mottola, David Santiago, and the speaker it is now possible to describe in some detail what happens physically when one approaches and crosses a region of space-time where classical general relativity predicts there should be an infinite red shift surface. This quantum critical physics provides a new perspective on a variety of enigmatic astrophysical phenomena including supernovae explosions, gamma ray bursts, positron emission, and dark matter.
- Research Organization:
- Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
- Sponsoring Organization:
- US Department of Energy (US)
- DOE Contract Number:
- W-7405-ENG-48
- OSTI ID:
- 15011619
- Report Number(s):
- UCRL-PROC-210580; TRN: US0501294
- Resource Relation:
- Conference: Presented at: Texas Conference on Relativistic Astrophysics, Stanford, CA (US), 12/12/2004--12/17/2004; Other Information: PBD: 8 Mar 2005
- Country of Publication:
- United States
- Language:
- English
Similar Records
Gravitational wave signatures of the absence of an event horizon: Nonradial oscillations of a thin-shell gravastar
PROCEEDINGS OF THE RIKEN BNL RESEARCH CENTER WORKSHOP ON LARGE SCALE COMPUTATIONS IN NUCLEAR PHYSICS USING THE QCDOC, SEPTEMBER 26 - 28, 2002.
Neutron Star Mergers Might Not Be the Only Source of r -process Elements in the Milky Way
Journal Article
·
Tue Dec 15 00:00:00 EST 2009
· Physical Review. D, Particles Fields
·
OSTI ID:15011619
+2 more
PROCEEDINGS OF THE RIKEN BNL RESEARCH CENTER WORKSHOP ON LARGE SCALE COMPUTATIONS IN NUCLEAR PHYSICS USING THE QCDOC, SEPTEMBER 26 - 28, 2002.
Technical Report
·
Thu Sep 26 00:00:00 EDT 2002
·
OSTI ID:15011619
+2 more
Neutron Star Mergers Might Not Be the Only Source of r -process Elements in the Milky Way
Journal Article
·
Sat Apr 20 00:00:00 EDT 2019
· The Astrophysical Journal (Online)
·
OSTI ID:15011619
+8 more